Galaxy-Scale Fountain Seen in Full GloryNovember 6, 2018
Infalling and Outflowing Gas Give More Complete Understanding of the Evolution of Galaxies
Astronomers have long theorized that fountains such as this continually recirculate a galaxy’s star-forming fuel. New Atacama Large Millimeter/submillimeter Array (ALMA)
observations of Abell 2597 show the first clear and compelling evidence for the simultaneous infalling and outflow of gas driven by a supermassive black hole. The researchers report their observations in the latest issue of the Astrophysical Journal.
“The supermassive black hole at the center of this giant galaxy acts like a mechanical ‘pump’ in a water fountain,” said Grant Tremblay, an astrophysicist at the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts, and lead author on the paper. “This is one of the first systems in which we find clear evidence for both cold molecular gas inflow toward the black hole and outflow or uplift from the jets that the black hole launches.”
According to the researchers, this entire system operates via a self-regulating feedback loop. The infalling material provides power for the fountain as it “drains” toward the central black hole, like water entering the pump of a fountain. This infalling gas then causes the black hole to ignite with activity, launching high-velocity jets of super-heated material that shoot out of the galaxy. As it travels, this material pushes out clumps and streamers of gas into the galaxy’s expansive halo, where it eventually rains back in on the black hole, triggering the entire process anew.
In total, about three billion solar mass
es of molecular gas is part of this fountain, forming a filamentary nebula that spans the innermost 100,000 light-years of the galaxy.
In an earlier study by the same authors published in the journal Nature, the researchers were able to verify the interconnection between the black hole and the galactic fountain by observing the region across a range of wavelengths, or portions of the spectrum. By studying the location and motion of molecules of carbon monoxide (CO) with ALMA, which shine brightly in millimeter-wavelength light, the researchers could measure the motion of the gas as it falls in toward the black hole.
Earlier data from the Multi-Unit Spectroscopic Explorer (MUSE) on ESO’s Very Large Telescope (VLT) revealed warm, ionized gas being expelled from the galaxy – essentially the plume of the fountain. The new ALMA observations found clumps of cold, molecular gas in precisely the same locations as the warm gas seen in the earlier observations.
“The unique aspect here is a very detailed coupled analysis of the source using data from ALMA and the MUSE instrument. The two facilities make for an incredibly powerful combination,” said Tremblay. “ALMA revealed the distribution and motions of the cold molecular gas clouds, and MUSE did the same for the warm ionized gas.”
The ALMA and MUSE data were combined with a new, ultra-deep observation of the cluster by NASA’s Chandra X-ray Observatory, revealing the hot phase of this fountain in exquisite detail, noted the researchers.
The observations also very convincingly support the hypothesis that the warm ionized and cold molecular nebula
s are one-in-the-same, with the warm ionized gas merely being the “shell” around the cold molecular cores that churn within this galaxy-scale fountain.
This multiwavelength approach offers an uncommonly complete picture of this system. “It’s like observing the rain cloud, rain, and puddle all at the same time,” noted Tremblay. While this is just one observation of one galaxy, the astronomers speculate that they may be observing a process that is common in galaxies and fundamental to their evolution.
The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.
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This research is presented in a paper titled “A Galaxy-scale Fountain of Cold Molecular Gas Pumped by a Black Hole” by G. Tremblay et al. in the Astrophysical Journal. [http://iopscience.iop.org/article/10.3847/1538-4357/aad6dd ]
The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of the European Southern Observatory (ESO), the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the Ministry of Science and Technology (MOST) in Taiwan and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).
ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA.